All Tables

Table 1: Previous variable star searches in NGC 6791.
Table 2: The observation log for each night and the limits of the field of view at the 3 different observatories.
Table 3: Pulsating, irregular and cataclysmic variables. V is the minimum brightness for CVs and irregular, the mean brightness for pulsating variables. T₀ is the time of maximum brightness for pulsating stars. Hereafter, the labels "k'' and "s'' indicate that the B-V color index is taken from Kaluzny & Rucinski (1995) or Stetson et al. (2003), respectively.
Table 4: Coordinates and light curve parameters of the contact binaries (W UMa systems, EW) belonging to NGC 6791. V is the brightness at maximum and T₀ is the time of the primary minimum.
Table 5: Eclipsing variables with well defined light curves. EA stands for a $\beta$ Per system, EB for a $\beta$ Lyr one. V is the brightness at maximum and T₀ is the time of the primary minimum. Also B4, V60 and 02461_8, whose parameters are reported in the Appendix, are possible cluster members. The last column shows the Cudworth membership probability (when available).
Table 6: Rotational variables belonging to the cluster. V is the mean brightness value. T₀ indicates the time of the maximum brightness. The last column shows the membership probability (when available) or our photometric membership. The two uncertain cases (V41 and V14) are also listed (see text).
Table 7: Long period variable stars that are likely members of NGC 6791 (ordered by increasing right ascension). Column 9 shows the membership probability (when available) or our photometric membership.
Table A.1: Pulsating, irregular and cataclysmic variables. V is the minimum brightness for CVs and irregular, the mean brightness for pulsating variables. T₀ is the time of maximum brightness for pulsating stars.
Table A.2: Contact binaries; V is the brightness at maximum and T₀ is the time of the primary minimum.
Table A.3: Eclipsing variables. V is the brightness at maximum and T₀ is the time of the primary minimum.
Table A.4: Rotational variables with a single-wave light curve. V is the mean brightness value. T₀ indicates the time of the maximum brightness.
Table A.5: Rotational variables with a double-wave light curve. V is the mean brightness value. T₀ indicates (one of) the times of maximum brightness.
Table A.6: Long period variable stars (ordered by increasing right ascension).